Coronal mass ejections (CMEs), including halo CMEs, can be
observed in interplanetary scintillation (IPS) data. To
optimize the information from radio source observations, we
model them using a time-dependent three-dimensional
tomography program. We depict this heliospheric model as a
series of "sky map" images that cover elongations extending
from 10 to 80 degrees. These IPS maps show CMEs observed
earlier in the LASCO coronagraph images with approximately
the same shapes and extents that were seen closer to the
Sun. Here, a series of these CME events, including halo
CMEs, are mapped as they move outward to distances as great
as 1 AU.

If you would like more information about this abstract, please
follow the link to http://casswww.ucsd.edu/solar/index.html.
This link was provided by the
author. When you follow it, you will leave the Web site for this
meeting; to return, you should use the Back comand on your
browser.